2010MNRAS.401..513J


Query : 2010MNRAS.401..513J

2010MNRAS.401..513J - Mon. Not. R. Astron. Soc., 401, 513-524 (2010/January-1)

Nuclear physics of reverse electron flow at pulsar polar caps.

JONES P.B.

Abstract (from CDS):

Protons produced in electromagnetic showers formed by the reverse electron flux are usually the largest component of the time-averaged polar cap open magnetic flux line current in neutron stars with positive corotational charge density. Although the electric field boundary conditions in the corotating frame are time independent, instabilities on both medium and short time-scales cause the current to alternate between states in which either protons or positrons and ions form the major component. These properties are briefly discussed in relation to nulling and microstructure in radio pulsars, pair production in an outer gap and neutron stars with high surface temperatures.

Abstract Copyright: © 2009 The Author. Journal compilation © 2009 RAS

Journal keyword(s): instabilities - plasmas - stars: neutron - pulsars: general

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 PSR J1933+2421 Psr 19 33 37.83 +24 36 39.6           ~ 157 0

Query : 2010MNRAS.401..513J

Basic data :
PSR J1933+2421 -- Pulsar
Other object types:
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Psr (PSR)
ICRS coord. (ep=J2000) :
19 33 37.83 +24 36 39.6 [ ] D 2006Sci...312..549K
FK4 coord. (ep=B1950 eq=1950) :
19 31 32.12 +24 30 05.7 [ ]
Gal coord. (ep=J2000) :
059.47821 +02.39421 [ ]
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Identifiers (3) :
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PSR J1933+2421 PSR B1931+24 PSR J1933+24

References (157 between 1850 and 2026) (Total 157)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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